The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.
# Object: 119067 # Created Sun Dec 22 02:06:52 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 24 observations of 24 # Arc: 5.96y # First observation: 2001/05/23 # Last observation: 2007/05/08 # Chi-squared of fit: 23.40 DOF: 42 RMS: 0.17 # Min/Max residuals: -0.44 0.62 # Exact a, adot, b, bdot, g, gdot: 1.460734E-05 2.126927E-02 -1.961190E-06 -2.542992E-03 2.319938E-02 -4.119101E-03 # Covariance matrix: 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 # lat0 lon0 xBary yBary zBary JD0 -2.425923 -118.085825 -0.002923 -0.043256 -1.018005 2452052.691053 # Heliocentric elements and errors Epoch: 2452052.5000 = 2001/05/23 Mean Anomaly: 275.15743 +/- 0.000 Argument of Peri: 305.63974 +/- 0.000 Long of Asc Node: 42.85288 +/- 0.000 Inclination: 7.22188 +/- 0.000 Eccentricity: 0.18963366 +/- 0.0000 Semi-Major Axis: 43.30714968 +/- 0.0000 Time of Perihelion: 2476585.4153 +/- 0.0 Perihelion: 35.09465621 +/- 0.0000 Aphelion: 51.51964315 +/- 0.0000 Period (y) 285.0018 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -20.74829946 +/- 0.0000 Ecliptic Y -38.88991854 +/- 0.0000 Ecliptic Z -1.82460371 +/- 0.0000 Ecliptic XDOT 0.00244072 +/- 0.0000 Ecliptic YDOT -0.00073975 +/- 0.0000 Ecliptic ZDOT -0.00027907 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.11640826 +/- 0.0000 Geocenter to KBO 43.10476795 +/- 0.0000 # Hcoef: 6.33
The following table shows the complete astrometric record for 119067. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (119067) followed by the observatory code and reference code for the source of the astrometry.
2001 05 23.19031 15 57 09.59 -22 55 14.5 21.9R 119067 807 Cd1817 2001 05 23.25457 15 57 09.27 -22 55 13.8 119067 807 Cd1817 2001 06 13.06841 15 55 29.50 -22 50 43.4 22.7R 119067 304 Cd1817 2001 06 13.19358 15 55 28.92 -22 50 41.8 119067 304 Cd1817 2002 05 12.02836 16 03 10.23 -23 20 36.6 119067 950 Cf4617 2002 05 12.07402 16 03 10.01 -23 20 36.1 119067 950 Cf4617 2002 05 12.11956 16 03 09.78 -23 20 35.5 119067 950 Cf4617 2002 05 13.03693 16 03 05.34 -23 20 25.6 119067 950 Cf4617 2002 05 13.10636 16 03 04.99 -23 20 24.7 119067 950 Cf4617 2003 04 29.49972 16 09 18.98 -23 45 12.3 23.2R 119067 568 Ch9866 2003 04 29.56677 16 09 18.69 -23 45 11.5 119067 568 Ch9866 2003 04 30.59832 16 09 14.09 -23 45 03.0 119067 568 Ch9866 2005 05 10.23777 16 18 59.93 -24 27 19.4 21.8R 119067 807 Cn5310 2005 05 10.30422 16 18 59.62 -24 27 18.9 119067 807 Cn5310 2005 05 11.16483 16 18 55.47 -24 27 11.6 119067 807 Cn5310 2005 08 08.05003 16 13 08.84 -24 12 44.2 22.0R 119067 807 Co3473 2005 08 08.16634 16 13 08.72 -24 12 43.3 119067 807 Co3473 2005 08 09.05617 16 13 07.82 -24 12 39.0 119067 807 Co3473 2006 04 26.24977 16 25 27.83 -24 50 01.9 21.6R 119067 807 Cr3798 2006 04 26.33397 16 25 27.51 -24 50 01.8 119067 807 Cr3798 2007 05 08.57739 16 30 02.44 -25 09 21.5 23.5R 119067 250 S~06HB 2007 05 08.58434 16 30 02.41 -25 09 21.5 119067 250 S~06HB 2007 05 08.59128 16 30 02.37 -25 09 21.4 119067 250 S~06HB 2007 05 08.59892 16 30 02.34 -25 09 21.4 119067 250 S~06HB
The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.
1 0.0000 0.00 -0.01 0.00 0.05
2 0.0002 0.00 0.02 0.00 -0.07
3 0.0572 0.00 0.28 0.00 0.09
4 0.0575 0.00 0.24 0.00 0.07
5 0.9688 0.00 -0.14 0.00 -0.00
6 0.9689 0.00 -0.07 0.00 0.00
7 0.9690 0.00 -0.15 0.00 0.10
8 0.9715 0.00 0.02 0.00 -0.09
9 0.9717 0.00 -0.08 0.00 0.05
10 1.9338 0.00 -0.22 0.00 -0.28
11 1.9340 0.00 -0.04 0.00 -0.03
12 1.9368 0.00 -0.27 0.00 -0.08
13 3.9645 0.00 0.04 0.00 0.08
14 3.9647 0.00 0.27 0.00 0.01
15 3.9671 0.00 0.16 0.00 -0.07
16 4.2104 0.00 -0.06 0.00 0.07
17 4.2107 0.00 0.08 0.00 0.32
18 4.2132 0.00 -0.08 0.00 0.09
19 4.9256 0.00 0.06 0.00 -0.10
20 4.9258 0.00 0.62 0.00 -0.44
21 5.9586 0.00 -0.20 0.00 -0.01
22 5.9586 0.00 -0.16 0.00 -0.05
23 5.9587 0.00 -0.27 0.00 0.00
24 5.9587 0.00 -0.18 0.00 -0.05
The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.
119067 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 43.350 43.350 43.350 ecceobj 0.192 0.192 0.192 incobj 7.229 7.229 7.229 qmin 34.607 34.609 34.607 qmax 53.594 53.585 53.609 amean 43.723 43.755 43.724 amin 43.182 43.190 43.167 amax 44.313 44.349 44.323 emean 0.179 0.177 0.176 emin 0.147 0.146 0.142 emax 0.210 0.210 0.210 imean 3.615 3.884 3.493 imin 0.028 0.306 0.226 imax 6.862 7.110 6.861 excite_mean 0.192 0.192 0.189 fracstop 1.000 1.000 1.000 cjmean 3.052 3.053 3.054 libcent 0 -180.0 -180.0 -180.0 libamp 0 -180.0 -180.0 -180.0 libcent 1 -180.0 -180.0 -180.0 libamp 1 -180.0 -180.0 -180.0 libcent 2 -180.0 -180.0 -180.0 libamp 2 -180.0 -180.0 -180.0 libcent 3 -180.0 -180.0 -180.0 libamp 3 -180.0 -180.0 -180.0 libcent 4 -180.0 -180.0 -180.0 libamp 4 -180.0 -180.0 -180.0 kozaimean 180.1 178.4 177.3 kozaiamp 180.0 180.0 180.0